Pulsars, transients and relativistic astrophysics

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First detections of the cataclysmic variable AE Aquarii in the near to far infrared with ISO and IRAS: Investigating the various possible thermal and non-thermal contributions

Astronomy & Astrophysics EDP Sciences 433:3 (2005) 1063-1077

Authors:

M Abada-Simon, J Casares, A Evans, S Eyres, R Fender, S Garrington, O de Jager, N Kuno, IG Martínez-Pais, D de Martino, H Matsuo, M Mouchet, G Pooley, G Ramsay, A Salama, B Schulz
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Jet Velocity in SS 433: Its Anticorrelation with Precession-Cone Angle and Dependence on Orbital Phase

Astrophysical Journal Letters 622 (2005) L129-L132

Authors:

KM Blundell, Michael G. Bowler
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Was the Narrow Line Seyfert 1 RGB J0044+193 ever radio loud?

Astronomy & Astrophysics EDP Sciences 433:2 (2005) 531-533

Authors:

TJ Maccarone, JCA Miller-Jones, RP Fender, GG Pooley
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The VLT-FLAMES Survey of Massive Stars: Observations in the Galactic Clusters NGC 3293, NGC 4755 and NGC 6611

(2005)

Authors:

CJ Evans, SJ Smartt, J-K Lee, DJ Lennon, A Kaufer, PL Dufton, C Trundle, A Herrero, S Simon-Diaz, A de Koter, W-R Hamann, MA Hendry, IK Hunter, MJ Irwin, AJ Korn, R-P Kudritzki, N Langer, MR Mokiem, F Najarro, AWA Pauldrach, N Przybilla, J Puls, RSI Ryans, MA Urbaneja, KA Venn, MR Villamariz
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The distribution of radio plasma in time and space.

Philos Trans A Math Phys Eng Sci 363:1828 (2005) 645-654

Abstract:

The influence of jet-ejected plasma has been an important theme of this meeting; I draw attention to the prevalence of jet-ejected plasma, in particular that which has not been properly accounted for in the past. There are three strands to this paper: important emission which is prominent only at the lowest radio frequencies; relic radio plasma which must exist if even the most basic aspects of radio source evolutionary models are correct; and evidence that some 'radio-quiet' quasars could be FR-I radio sources.
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